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Recycled Pulsars: Spins, Masses and Ages

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arxiv 1606.05117 v1 pith:MJKU23V2 submitted 2016-06-16 astro-ph.SR astro-ph.HE

Thomas M. Tauris This is my paper · ORCID
classification astro-ph.SRastro-ph.HE
keywords quantitiesbinarymassespulsarsrecycledaffectedagesb-fields
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Recycled pulsars are mainly characterized by their spin periods, B-fields and masses. All these quantities are affected by previous interactions with a companion star in a binary system. Therefore, we can use these quantities as fossil records and learn about binary evolution. Here, I briefly review the distribution of these observed quantities and summarize our current understanding of the pulsar recycling process.

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Cited by 1 Pith paper

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  1. Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties

    astro-ph.HE 2019-08 conditional novelty 5.0 of 10

    Predictions of BHNS kilonova and afterglow light curves show that low-mass neutron stars produce brighter EM counterparts and that the blue B-band deficit can distinguish BHNS from NSNS mergers.

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